UVCS MISSION LOG ---------------- Date: 14 January 2008 ----- Last revision: 29 January 2008 (Wu) -------------- File Name: 2008.01.15.a.log ---------- Compiled by: Y.-K. Ko ------------ UVCS Activity: South Coronal Hole OVI Observation for -------------- 15 - 16 January 2008 Load South Coronal Hole OVI Observation for 16 - 17 January 2008 Load OVI Detector Diagnostic for 17 January 2008 SOHO Activity: -------------- EOF Staff: M. P. Miralles: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo: Planner R. Wu Command file: 08.01.14.14:23:37.cmd.log Activity: --------- 1) South Polar Coronal Hole OVI Observations Sequence: 08.01_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0 SCI_SPEC: Characterization of a polar coronal hole. Goal is to measure the properties of a polar coronal hole. In particular we are interested in the coronal conditions (intensities and line widths for HI Ly-alpha and OVI 1032/1037) as a function of height and latitude. We will compare these properties with the ones found in non-polar coronal holes. Roll positions are VL-corrected for PA=180 degrees. OBS_PROG: Primary: Sensitivity Sub Obj: Spatial Coverage SCI_OBJ: Plasma Properties...Proton and Ion Temperatures OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2008.01.15.16:05 end: 2008.01.16.15:06 ONUMs = 23974 (317 exps) 23975 (346 exps) Instrument configuration: - Pointing: Sun center - Spacecraft Roll: 180 Degrees - Roll: 174.38 Degrees (17739) - Mirror/Occulter: 2.4 Ro 1.5 mm overocculting - LYA Slit: 100 um - OVI Slit: 75 um - LYA GRTPOS: 100000 - OVI GRTPOS: 217000 - OVI MCP Voltage: 200 - OVI mask: OVI_EclipSyn_215 in slot 2 Fits Files: q08.01.15.16:05:06.ovi.dat GAP between 01/15/08|18:53:55( 2750) and 01/15/08|18:56:21( 2979) q08.01.16.03:06:26.ovi.dat GAP between 01/16/08|09:36:44( 5647) and 01/16/08|09:37:50( 5744) GAP between 01/16/08|14:29:09( 968) and 01/16/08|14:31:26( 1187)